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Jet Properties of GeV-selected Radio-loud Narrow-line Seyfert 1 Galaxies and Possible Connection to Their Disk and Corona

  • Authors: Xiao-Na Sun, Jin Zhang, Da-Bin Lin, Zi-Wei Xue, En-Wei Liang, and Shuang-Nan Zhang

Sun et al. 2015 The Astrophysical Journal 798 43.

  • Provider: AAS Journals

Caption: Figure 8.

(a) Jet luminosity (Ljet) as a function of the corona luminosity (Lcorona) for 1H 0323+342 and 3C 273. The jet luminosities are taken from the same energy band as the corona emission. Ljet and Lcorona of 1H 0323+342 are taken from 1016 Hz to 150 keV. The data of 3C 273 are taken from Grandi & Palumbo (2004) in energy band of 2–10 keV. (b) δ as a function of Lcorona for 1H 0323+342.

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